What's astonishing is that both Ikeya and Murakami did it the old-fashioned way: by looking into the eyepiece of a telescope! Visual comet discoveries have become a rarity in this age of powerful professional surveys and digital imaging techniques.
Brian G. Marsden (Minor Planet Center) has calculated a preliminary orbit for the comet, designated C/2010 V1. It is moving in a parabolic orbit and is just past perihelion at 1.7 astronomical units from the Sun (that is, well outside the orbit of Mars). So while this comet won't be getting any brighter in the coming weeks, it should stay within reach of binoculars as it moves slowly southeastward across Virgo.
On November 4th, J. J. Gonzales in Spain and Carl Hergenrother in Arizona called it roughly magnitude 7.5 in their binoculars, while Alan Hale in New Mexico put it at 9.0. To all three observers, it resembled a fuzzy round glow with no tail.
The following ephemeris gives the comet's coordinates (equinox 2000.0) at 0 hours Universal Time on selected dates, aling with its angular elongation from the Sun.
|Nov. 5||12 38.0||-02 26||32.6|
|Nov. 7||12 43.1||-03 06||33.2|
|Nov. 9||12 48.2||-03 47||33.8|
|Nov. 11||12 53.3||-04 27||34.4|
|Nov. 13||12 58.3||-05 06||35.0|
|Nov. 15||13 03.4||-05 46||35.6|
Be sure to check the online version of this AstroAlert on Sky & Telescope's website for updates when the orbit is improved:
Also stay tuned to our website's observing highlights. Good luck, and clear skies!
Senior Contributing Editor
Sky & Telescope